Normalizing the Temperature Function of Clusters of Galaxies

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Temperature Profiles of Nearby Clusters of Galaxies

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X iv : a st ro - p h / 96 10 14 7 v 3 6 D ec 1 99 7 Normalizing the Temperature Function of Clusters of Galaxies

We reexamine the constraints which can be robustly obtained from the observed temperature function of X-ray cluster of galaxies. The cluster mass function has been thoroughly studied in simulations and analytically, but a direct simulation of the temperature function is presented here for the first time. Adaptive hydrodynamic simulations using the cosmological Moving Mesh Hydro code of Pen (199...

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1998

ISSN: 0004-637X,1538-4357

DOI: 10.1086/305514